On Friday, November 1, 2019 at 1:43:50 AM UTC-5, Alan Grayson wrote: > > > > On Friday, November 1, 2019 at 12:24:21 AM UTC-6, Philip Thrift wrote: >> >> >> >> On Thursday, October 31, 2019 at 4:33:29 PM UTC-5, Tomasz Rola wrote: >>> >>> On Thu, Oct 31, 2019 at 09:56:01AM -0700, Philip Thrift wrote: >>> > >>> > >>> > >>> http://backreaction.blogspot.com/2019/10/the-crisis-in-physics-is-not-only-about.html >>> >>> >>> Yeah. Interesting article and comments are worth a read, too. Perhaps >>> the problem she described stems from limits in human cognition. >>> >>> quote: >>> >>> "But even if you don’t care what’s up with strings and multiverses, >>> you should worry about what is happening here. The foundations of >>> physics are the canary in the coal mine." >>> >>> end quote >>> >>> Indeed. I could not care less about strings and multiverses (unless I >>> can see a device making use of those theories), but I am a bit >>> worried. >>> >>> -- >>> Regards, >>> Tomasz Rola >>> >>> -- >>> ** A C programmer asked whether computer had Buddha's nature. ** >>> ** As the answer, master did "rm -rif" on the programmer's home ** >>> ** directory. And then the C programmer became enlightened... ** >>> ** ** >>> ** Tomasz Rola mailto:[email protected] >> >> >> >> >> There are all these projects, like "It from Qubit" (emergence of >> spacetime from quantum entanglement, Simons Foundation and Perimeter >> Institute) from 3 years ago, but they all seem to fizzle out and produce >> nothing. >> >> @philipthrift >> > > They get more and more expensive, but many don't fizzle out; such as the > Kepler spacecraft which has found around 2000 planets, and many other > scientific spacecraft such as Galileo, Juno, Cassini, as well as the > several spacecraft that have mapped the CMBR in ever greater detail. I > could go on. Maybe she needs a cold shower. AG >
This has nothing to do with money for bigger and better instruments (bigger is better, right?). It has to do with the fizzle out of fundamental theory. >From the last conference: The 2019 annual meeting of It from Qubit: Simons Collaboration on Quantum Fields, Gravity, and Information will be devoted to recent developments at the interface of fundamental physics and quantum information theory, spanning topics such as chaos and thermalization in many-body systems and their realization in quantum gravity; traversable wormholes and their information-theoretic implications; calculable lower-dimensional models of quantum gravity; the entanglement structure of semi-classical states in quantum gravity; complexity in field theory and gravity; the black-hole information puzzle; and applications of near-term quantum devices to problems in high-energy physics. Abstracts Matthew Headrick Brandeis University Bit Threads and Holographic Entropy Inequalities Entanglement entropies in holographic theories as computed by the Ryu-Takayanagi formula are known to obey many inequalities beyond those required of general quantum states. Headrick will explain how these special properties can be understood in the language of bit threads and what they might imply for the entanglement structure of the underlying states. Don Marolf University of California, Santa Barbara The Universal Structure of Holographic Quantum Codes Don Marolf argues that the structure of holographic quantum codes is related to a simple splitting into two parts of the bulk gravitational path integrals. In particular, treating the bulk as an effective field theory means that we are given an effective Lagrangian LΛ associated with a cut-off energy scale Λ. We show that aspects of the code are then determined by classical computations involving LΛ, while the path integral over fluctuations below the scale Λ determines the states to be encoded. As a result, in each superselection sector, all such codes turn out to have flat entanglement spectrum up to corrections of order G (i.e., up to corrections of order G2 times the leading term, which is itself of order 1/G). This statement holds for any LΛ, no matter what higher derivative terms it may contain. Marolf also comments on other applications of fixed-area states or more generally of states with fixed geometric entropy. Vijay Balasubramanian University of Pennsylvania Quantum Complexity of Time Evolution with Chaotic Hamiltonians Balasubramanian studies the quantum complexity of time evolution in large-N chaotic systems, with the SYK model as our main example. This complexity is expected to increase linearly for exponential time prior to saturating at its maximum value and is related to the length of minimal geodesics on the manifold of unitary operators that act on Hilbert space. Using the Euler-Arnold formalism, Balasubramanian demonstrates that there is always a geodesic between the identity and the time evolution operator e−iHt, whose length grows linearly with time. This geodesic is minimal until there is an obstruction to its minimality, after which it can fail to be a minimum either locally or globally. Balasubramanian identifies a criterion — the Eigenstate Complexity Hypothesis (ECH) — which bounds the overlap between off-diagonal energy eigenstate projectors and the k-local operators of the theory — and uses it to show that the linear geodesic will at least be a local minimum for exponential time. He shows numerically that the large-N SYK model (which is chaotic) satisfies ECH and thus has no local obstructions to linear growth of complexity for exponential time, as expected from holographic duality. In contrast, he also studies the case with N=2 fermions (which is integrable) and finds short-time linear complexity growth followed by oscillations. His analysis relates complexity to familiar properties of physical theories, like their spectra and the structure of energy eigenstates, and has implications for the hypothesized computational complexity class. Christine Muschik University of Waterloo How to Simulate Lattice Gauge Theories on Quantum Computers Gauge theories are fundamental to our understanding of interactions between the elementary constituents of matter as mediated by gauge bosons. Muschik will talk about proposals for quantum simulations of gauge theories and their recent implementation on a trapped ion quantum computer. Considering one-dimensional quantum electrodynamics, Muschik and collaborators addressed the real-time evolution of particle-antiparticle pair production in a digital quantum simulation [Nature 534, 516-519 (2016)] as well as hybrid classical-quantum algorithms [Nature 569, 355 (2019)] to simulate equilibrium problems. Muschik will also discuss recent results on extending this work beyond one spatial dimension. Alex Maloney McGill University De Sitter Quantum Gravity in 2 and 3 Dimensions Maloney will discuss aspects of JT gravity in two-dimensional nearly de Sitter (dS) space-time and pure de Sitter quantum gravity in three dimensions. Both are essentially topological theories of gravity where it is possible to study precisely the wave function of the universe following the Hartle-Hawking construction. The wave function can be computed by analytic continuation to Euclidean AdS, rather than the sphere; this allows us to compute all of the perturbative and (in two dimensions) nonperturbative corrections to the wave function and to formulate the theory as a Matrix integral and provides a connection with the quantization of the moduli space of Riemann surfaces. Stephen Shenker Stanford University Black Holes, Random Matrices, Baby Universes and D-branes The energy spectrum of generic large AdS black holes is discrete because their entropy is finite. The explanation for this is clear from the boundary field theory point of view in AdS/CFT — it is just the discrete spectrum of a bound quantum system. But the explanation for this discreteness from the bulk gravitational point of view remains a mystery. We will discuss some progress on a simpler related problem: the gravitational origin of the statistical properties of this discrete spectrum in an ensemble of quantum systems. Because black holes are quantum chaotic systems, we expect these statistics to be described by random matrix ensembles. Shenker’s analysis will focus on the simple model black hole described by the Sachdev-Ye-Kitaev (SYK) model and, in particular, on its low-energy limit, Jackiw-Teitelboim (JT) gravity. We will be led to consider an asymptotic expansion described by space-time manifolds with an arbitrary number of handles and its completion by an analog of D-branes. We will close by discussing some of the questions this analysis raises — based on joint work with Phil Saad and Douglas Stanford. Jonathan Oppenheim University College London A Post-Quantum Theory of Classical Gravity? Oppenheim presents a consistent theory of classical gravity coupled to quantum field theory. The dynamics are linear in the density matrix, completely positive and trace preserving, and reduce to Einstein’s equations in the classical limit. The constraints of general relativity are imposed as a symmetry on the equations of motion. The assumption that gravity is classical necessarily modifies the dynamical laws of quantum mechanics; the theory must be fundamentally stochastic involving finite-sized and probabilistic jumps in space-time and in the quantum field. Nonetheless, the quantum state of the system can remain pure, conditioned on the classical degrees of freedom. The measurement postulate of quantum mechanics is not needed since the interaction of the quantum degrees of freedom with classical space-time necessarily causes collapse of the wave function. More generally, Oppenheim derives a form of classical-quantum dynamics using a noncommuting divergence, which has as its limit deterministic classical Hamiltonian evolution and which doesn’t suffer from the pathologies of the semi-classical theory. The theory can be regarded as fundamental or as an effective theory of QFT in curved space where back-reaction is consistently accounted for. @philipthrift -- You received this message because you are subscribed to the Google Groups "Everything List" group. To unsubscribe from this group and stop receiving emails from it, send an email to [email protected]. To view this discussion on the web visit https://groups.google.com/d/msgid/everything-list/1741dbf4-39be-4ff2-bbda-ef82082f8b40%40googlegroups.com.
